Energy Distribution in 2d Stringy Black Hole Backgrounds
General Relativity and Quantum Cosmology
2009-11-10 v2 Astrophysics
High Energy Physics - Theory
Abstract
We utilize Moller's and Einstein's energy-momentum complexes in order to explicitly evaluate the energy distributions associated with the two-dimensional "Schwarzschild" and "Reissner-Nordstrom" black hole backgrounds. While Moller's prescription provides meaningful physical results, Einstein's prescription fails to do so in the aforementioned gravitational backgrounds. These results hold for all two-dimensional static black hole geometries. The results obtained within this context are exploited in order Seifert's hypothesis to be investigated.
Cite
@article{arxiv.gr-qc/0303009,
title = {Energy Distribution in 2d Stringy Black Hole Backgrounds},
author = {Elias C. Vagenas},
journal= {arXiv preprint arXiv:gr-qc/0303009},
year = {2009}
}
Comments
17 pages, LaTeX, v2: acknowledgements added, to appear in Int.J.Mod.Phys.A